Axionlike Dark Matter Model Involving Two-Phase Structure and Two-Particle Composites (Dimers)
arXiv:2309.03290 · doi:10.1103/PhysRevD.108.123030
Abstract
Within the self-gravitating Bose-Einstein condensate (BEC) model of dark matter (DM), we argue that the axionlike self-interaction of ultralight bosons ensures the existence of both rarefied and dense phases in the DM halo core of (dwarf) galaxies. In fact, this stems from two independent solutions of the Gross-Pitaevskii equation corresponding to the same model parameters. For a small number of particles, this structure disappears along with the gravitational interaction, and the Gross-Pitaevskii equation reduces to the stationary sine-Gordon equation, the one-dimensional antikink solution of which mimics a single-phase DM radial distribution in the halo core. Quantum mechanically, this solution corresponds to a zero-energy bound state of two particles in a closed scattering channel formed by the domain-wall potential with a finite asymptotics. To produce a two-particle composite with low positive energy and a finite lifetime, we appeal to the resonant transition of one asymptotically free particle of a pair from an open channel (with a model scattering potential) to the closed channel. Using the Feshbach resonance concept, the problem of two-channel quantum mechanics is solved in the presence of a small external influence which couples the two channels, and an analytical solution is obtained in the first approximation. Analyzing the dependence of scattering data on interaction parameters, we reveal a long-lived two-particle composite (dimer) possessing a lifetime of millions of years. This result is rather surprising and supposes important implications of dimers' being involved in forming large DM structures. It is shown that the dimers' appearance is related with the regime of infinite scattering length due to resonance. The revealed dependence of the DM scattering length on the parameters of interactions can theoretically justify variation of in the DM dominated galaxies.
16 pages, 7 figures; v2: few refs. added, takes into account referee's remarks; to appear in Phys. Rev. D
References in corpus (13)
- Bose-Einstein Condensation of Dark Matter Axions
- The dark-matter axion mass
- A High Resolution Search for Dark-Matter Axions
- Bose-Einstein condensation of dark matter solves the core/cusp problem
- Three-particle quantization condition in a finite volume: 1. The role of the three-particle force
- Cosmic structures via Bose Einstein condensation and its collapse
- Axions: Bose Einstein Condensate or Classical Field?
- Gravitational waves and kicks from the merger of unequal mass, highly compact boson stars
- Gravitational collapse of Bose-Einstein condensate dark matter halos
- Phases of the Bose-Einstein condensate dark matter model with both two- and three-particle interactions
- Partition Function of the Bose-Einstein Condensed Dark Matter and the Modified Gross-Pitaevskii Equation
- New Deformed Heisenberg Algebra from the -Deformed Model of Dark Matter
- Bose-Einstein Condensate Dark Matter That Involves Composites